PIC simulations of oblique shocks in turbulent plasma show that pre-existing 15% compressive turbulence produces a shorter hotter foreshock and more numerous higher-energy non-thermal electrons.
Production of Magnetic Turbulence by Cosmic Rays Drifting Upstream of Supernova Remnant Shocks , volume =
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PIC simulations of nonrelativistic high-Mach-number oblique shocks propagating in a turbulent medium
PIC simulations of oblique shocks in turbulent plasma show that pre-existing 15% compressive turbulence produces a shorter hotter foreshock and more numerous higher-energy non-thermal electrons.